Derivation of stefan boltzmann law from planck's law .
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Stefan-Boltzmann Law. Specifically, this law states that:The total energy radiated per unit surface area of a black body across all wavelengths per unit time is directly proportional to the fourth power of the black body’s thermodynamic temperature T.Expressed in appropriate terms, mathematically speaking: Eq. 1, whereis theEmissive Power(also known as the black-body irradiance), is the Stefan-Boltzmann constant, 5,67 × 10-8 W/ m2 K4, and Tis the absolute temperature of the emitting surface
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